Dark matter detectors are designed to be quiet. Eventually they become quiet enough to hear something else.
The background that remains
Shielding and underground sites reduce cosmic rays and radioactivity. Neutrinos still pass through almost everything, and occasionally they interact.
Not a wall
The “neutrino floor” is not a point where experiments stop. It is a region where additional information becomes necessary.
Designing for ambiguity
Future detectors may use target materials, timing, and direction to decide whether an event looks more like dark matter or a known neutrino source.






